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  • 1
    Online Resource
    Online Resource
    Advances in Solar Physics : Proceedings of the Seventh European Meeting on Solar Physics Held in Catania, Italy, 11-15 May 1993 (1994)
    Berlin, Heidelberg : Springer Berlin Heidelberg
    Details
    UID:
    gbv_749242248
    Format: 1 Online-Ressource (XVII, 338 p)
    Edition: Springer eBook Collection. Physics and Astronomy
    ISBN: 9783540484202 , 9783540580416
    Series Statement: Lecture Notes in Physics 432
    Content: This book begins with a very readable survey "The Sun Today" by J.-C. Pecker. It is followed by thorough reviews from leading experts covering theory and observations. The focus shifts from the solar core, studied via neutrino emissions and helioseismology, through the interface regions where it is believed the large-scale magnetic fields are generated, to the corona, where most of the high temperature phenomena characteristic of this region may be studied directly. As energetic particles play such a vigorous role in this part of the sun, a separate session was devoted to their transport and storage in the corona
    Content: The Sun today -- Recent results from helioseismology -- The structure of the solar core -- New sub-barrier nuclear fusion cross sections as a possible solution to the solar neutrino problem -- Helioseismic evidence for mixing in the radiative interior -- Microscopic settling and turbulent diffusion induced by rotation in the sun -- Mean-field theory of the solar dynamo -- Hydrodynamical simulations of the solar dynamo -- The asymmetric behaviour of solar activity -- On the possibility of supergiant stable flows in the convection zone of the sun -- Stellar dynamos -- On magnetic fields, rossby numbers and dynamo action in late-type stars -- The magnetic field of the solar corona -- The control of the corona by the convective zone magnetic fields -- Line-tying in a gravitationally stratified atmosphere -- Magnetic fields surrounding coronal holes -- Coronal heating mechanisms -- Coronal heating via nanoflares -- Magnetic structures of the intermediate corona -- Oscillations in quiescent prominences -- Pressure diagnostics of coronal loops observed by NIXT -- Quiet sun from multifrequency radio observations on RATAN-600 -- Frequency spectra of solar microwave bursts associated with coronal mass ejections -- Observations of high-energy (E?10 MeV) gamma-rays with the PHEBUS instrument -- Observational characteristics of explosive events -- Plasma physics of explosive phenomena -- A search for small solar flares with BATSE -- Solar flares and laboratory experiments -- Particle acceleration and radiation generation by nonlinear mode-mode coupling processes in the solar corona -- A fast mechanism for the acceleration of solar energetic particles in solar flares -- Acceleration and storage of energetic particles in the solar corona -- Electromagnetic signatures of particle acceleration and propagation -- Proton acceleration in long duration flares -- Signatures of proton beams in the Ly? profile: Sensitivity of the diagnostics -- Ground - based instrumentation -- Space instrumentation -- The Yohkoh mission: Instruments and recent results -- High resolution solar observations: Spectropolarimetry with THEMIS -- Conference summary
    Additional Edition: ISBN 9783540580416
    Language: English
    DOI: 10.1007/3-540-58041-7
    URL: Volltext
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    Stabi Berlin
    UB Potsdam
  • 2
    Online Resource
    Online Resource
    Advances in Solar Physics : Proceedings of the Seventh European Meeting on Solar Physics Held in Catania, Italy, 11–15 May 1993 (1994)
    Berlin, Heidelberg :Springer Berlin Heidelberg :
    Details
    UID:
    almafu_9959186124802883
    Format: 1 online resource (XVII, 338 p.)
    Edition: 1st ed. 1994.
    Edition: Online edition Springer Lecture Notes Archive ; 041142-5
    ISBN: 3-540-48420-5
    Series Statement: Lecture Notes in Physics, 432
    Content: This book begins with a very readable survey "The Sun Today" by J.-C. Pecker. It is followed by thorough reviews from leading experts covering theory and observations. The focus shifts from the solar core, studied via neutrino emissions and helioseismology, through the interface regions where it is believed the large-scale magnetic fields are generated, to the corona, where most of the high temperature phenomena characteristic of this region may be studied directly. As energetic particles play such a vigorous role in this part of the sun, a separate session was devoted to their transport and storage in the corona.
    Note: Bibliographic Level Mode of Issuance: Monograph , The Sun today -- Recent results from helioseismology -- The structure of the solar core -- New sub-barrier nuclear fusion cross sections as a possible solution to the solar neutrino problem -- Helioseismic evidence for mixing in the radiative interior -- Microscopic settling and turbulent diffusion induced by rotation in the sun -- Mean-field theory of the solar dynamo -- Hydrodynamical simulations of the solar dynamo -- The asymmetric behaviour of solar activity -- On the possibility of supergiant stable flows in the convection zone of the sun -- Stellar dynamos -- On magnetic fields, rossby numbers and dynamo action in late-type stars -- The magnetic field of the solar corona -- The control of the corona by the convective zone magnetic fields -- Line-tying in a gravitationally stratified atmosphere -- Magnetic fields surrounding coronal holes -- Coronal heating mechanisms -- Coronal heating via nanoflares -- Magnetic structures of the intermediate corona -- Oscillations in quiescent prominences -- Pressure diagnostics of coronal loops observed by NIXT -- Quiet sun from multifrequency radio observations on RATAN-600 -- Frequency spectra of solar microwave bursts associated with coronal mass ejections -- Observations of high-energy (E?10 MeV) gamma-rays with the PHEBUS instrument -- Observational characteristics of explosive events -- Plasma physics of explosive phenomena -- A search for small solar flares with BATSE -- Solar flares and laboratory experiments -- Particle acceleration and radiation generation by nonlinear mode-mode coupling processes in the solar corona -- A fast mechanism for the acceleration of solar energetic particles in solar flares -- Acceleration and storage of energetic particles in the solar corona -- Electromagnetic signatures of particle acceleration and propagation -- Proton acceleration in long duration flares -- Signatures of proton beams in the Ly? profile: Sensitivity of the diagnostics -- Ground — based instrumentation -- Space instrumentation -- The Yohkoh mission: Instruments and recent results -- High resolution solar observations: Spectropolarimetry with THEMIS -- Conference summary. , English
    In: Springer eBooks
    Additional Edition: ISBN 3-540-58041-7
    Language: English
    DOI: 10.1007/3-540-58041-7
    URL: http://dx.doi.org/10.1007/3-540-58041-7
    Library Location Call Number Volume/Issue/Year Availability
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    FU Berlin
    Charité
  • 3
    Online Resource
    Online Resource
    Accretion Disks and Magnetic Fields in Astrophysics : Proceedings of the European Physical Society Study Conference, Held in Noto (Sicily), Italy, June 16–21, 1988 (1989)
    Dordrecht : Springer Netherlands
    Details
    UID:
    b3kat_BV042415019
    Format: 1 Online-Ressource (XX, 297 p)
    ISBN: 9789400924017 , 9789401075817
    Series Statement: Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews 156
    Note: The present volume collects the review and contributed papers presented at the Europhysics Study Conferenee "Accretion Disks and Magnetic Fields in Astrophysics" held in Noto, Sicily, Italy, from 16 to 21 June 1988, under the High Patronage of the President of the Italian Republie and the local patronage of the Centro di Studi Superiori e di Ricerche (Center for Advanced Study and Research), a scientific institution supported by the City of Nota and the University of Catania. The attendance to the Conference was limited to about fifty selected participants from Canada, China, Denmark, France, Germany F.R., Italy, Japan, the Netherlands, Spain, Switzerland, United Kingdom and United States, in order to give the meeting the character and appearance of a real workshop, whose main aim was to highlight a varied but somewhat unified picture of the interaction, in different astrophysical systems, of rotation, turbulence and magnetism, with specific reference to accretion disks
    Language: English
    Keywords: Akkretion ; Astrophysik ; Magnetfeld ; Astrophysik ; Konferenzschrift
    DOI: 10.1007/978-94-009-2401-7
    URL: Volltext
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    TU Berlin
  • 4
    Online Resource
    Online Resource
    Diazepam elimination in premature and full term infants, and children (1973)
    Berlin : Kooperation de Gruyter
    Details
    UID:
    edochu_18452_13727
    ISSN: 1619-3997 , 1619-3997
    Content: Peer Reviewed
    In: Journal of Perinatal Medicine - Official Journal of the WAPM, : de Gruyter, 2009, 1,1973,2, Seiten 133-141, 1619-3997
    Language: Undetermined
    DOI: 10.1515/jpme.1973.1.2.133
    DOI: 10.18452/13075
    URN: urn:nbn:de:kobv:11-100167511
    URL: Volltext  (kostenfrei)
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    Online Resource
    Fulltext
    HU Berlin
  • 5
    Online Resource
    Online Resource
    Accretion Disks and Magnetic Fields in Astrophysics : Proceedings of the European Physical Society Study Conference, Held in Noto (Sicily), Italy, June 16-21, 1988 (1989)
    Dordrecht :Springer Netherlands :
    Details
    UID:
    almahu_9949199261602882
    Format: XX, 297 p. , online resource.
    Edition: 1st ed. 1989.
    ISBN: 9789400924017
    Series Statement: Astrophysics and Space Science Library, 156
    Note: The Relevance of Magnetic Fields to Stars and Accretion Disks -- Dynamo Processes in Stars -- The Nonlinear Breakup of the Sun's Toroidal Field -- Nonlinear Rossby-Alfven Global Waves on the Surface of a Rotating Sphere -- Accretion Discs in Theory and Practice -- Instabilities in Dwarf Nova Accretion Disks -- Accretion and Particle Acceleration by Spiral Shock Waves -- Magnetohydrodynamic Flows in Accretion Disks and Jets -- Slender Fluxtubes in Accretion Disks -- Magnetic Fields in the Accretion Disks of Cataclysmic Variables -- Accretion Discs and Magnetic Cataclysmic Variables -- Radio Emission of Dwarf Novae -- Jets and Magnetic Fields -- Hydromagnetic Flows from Rapidly Rotating Compact Objects and the Formation of Relativistic Jets -- Three Dimensional Simulation of Accretion Disks with Smoothed Particle Hydrodynamics -- The Early Stages of Star Formation -- Accretion Disks and Jets in Protostellar Systems -- Massive Cloud of Active Star Formation and the Spinning Streamer as Angular Momentum Drain -- Monte Carlo Simulation of H2 Formation by Cosmic Rays: Effect of the Grain Model -- Magnetic Field Generation during Galaxy Formation -- Numerical Simulation of Weakly Magnetized Propagating Slab Jets -- Numerical Simulation of Mass Outflows from Star Forming Regions -- Outflows from Active Galactic Nuclei -- Formation of Radio Jets and Lobes, and Enhanced Energy Liberation at AGN's -- Relativistic Radiative Transfer using Moment Formalism -- Fluid Models for Relativistic Warm Plasmas -- Magnetic Fields in the Central Engines of Active Galactic Nuclei -- Time Variability of the X-Ray Emission from Seyfert Galaxies -- Slim Accretion Discs -- Summary of the Conference: Stars -- Conference Summary: Active Galactic Nuclei.
    In: Springer Nature eBook
    Additional Edition: Printed edition: ISBN 9789401075817
    Additional Edition: Printed edition: ISBN 9780792302957
    Additional Edition: Printed edition: ISBN 9789400924024
    Language: English
    DOI: 10.1007/978-94-009-2401-7
    URL: https://doi.org/10.1007/978-94-009-2401-7
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    HU Berlin
  • 6
    Online Resource
    Online Resource
    Advances in Solar Physics : Proceedings of the Seventh European Meeting on Solar Physics Held in Catania, Italy, 11–15 May 1993 (1994)
    Berlin, Heidelberg :Springer Berlin Heidelberg :
    Details
    UID:
    edoccha_9959186124802883
    Format: 1 online resource (XVII, 338 p.)
    Edition: 1st ed. 1994.
    Edition: Online edition Springer Lecture Notes Archive ; 041142-5
    ISBN: 3-540-48420-5
    Series Statement: Lecture Notes in Physics, 432
    Content: This book begins with a very readable survey "The Sun Today" by J.-C. Pecker. It is followed by thorough reviews from leading experts covering theory and observations. The focus shifts from the solar core, studied via neutrino emissions and helioseismology, through the interface regions where it is believed the large-scale magnetic fields are generated, to the corona, where most of the high temperature phenomena characteristic of this region may be studied directly. As energetic particles play such a vigorous role in this part of the sun, a separate session was devoted to their transport and storage in the corona.
    Note: Bibliographic Level Mode of Issuance: Monograph , The Sun today -- Recent results from helioseismology -- The structure of the solar core -- New sub-barrier nuclear fusion cross sections as a possible solution to the solar neutrino problem -- Helioseismic evidence for mixing in the radiative interior -- Microscopic settling and turbulent diffusion induced by rotation in the sun -- Mean-field theory of the solar dynamo -- Hydrodynamical simulations of the solar dynamo -- The asymmetric behaviour of solar activity -- On the possibility of supergiant stable flows in the convection zone of the sun -- Stellar dynamos -- On magnetic fields, rossby numbers and dynamo action in late-type stars -- The magnetic field of the solar corona -- The control of the corona by the convective zone magnetic fields -- Line-tying in a gravitationally stratified atmosphere -- Magnetic fields surrounding coronal holes -- Coronal heating mechanisms -- Coronal heating via nanoflares -- Magnetic structures of the intermediate corona -- Oscillations in quiescent prominences -- Pressure diagnostics of coronal loops observed by NIXT -- Quiet sun from multifrequency radio observations on RATAN-600 -- Frequency spectra of solar microwave bursts associated with coronal mass ejections -- Observations of high-energy (E?10 MeV) gamma-rays with the PHEBUS instrument -- Observational characteristics of explosive events -- Plasma physics of explosive phenomena -- A search for small solar flares with BATSE -- Solar flares and laboratory experiments -- Particle acceleration and radiation generation by nonlinear mode-mode coupling processes in the solar corona -- A fast mechanism for the acceleration of solar energetic particles in solar flares -- Acceleration and storage of energetic particles in the solar corona -- Electromagnetic signatures of particle acceleration and propagation -- Proton acceleration in long duration flares -- Signatures of proton beams in the Ly? profile: Sensitivity of the diagnostics -- Ground — based instrumentation -- Space instrumentation -- The Yohkoh mission: Instruments and recent results -- High resolution solar observations: Spectropolarimetry with THEMIS -- Conference summary. , English
    In: Springer eBooks
    Additional Edition: ISBN 3-540-58041-7
    Language: English
    DOI: 10.1007/3-540-58041-7
    URL: http://dx.doi.org/10.1007/3-540-58041-7
    Library Location Call Number Volume/Issue/Year Availability
    BibTip Others were also interested in ...
    Online Resource
    Open Access Request
    Charité
  • 7
    Online Resource
    Online Resource
    Advances in Solar Physics : Proceedings of the Seventh European Meeting on Solar Physics Held in Catania, Italy, 11–15 May 1993 (1994)
    Berlin, Heidelberg :Springer Berlin Heidelberg :
    Details
    UID:
    edocfu_9959186124802883
    Format: 1 online resource (XVII, 338 p.)
    Edition: 1st ed. 1994.
    Edition: Online edition Springer Lecture Notes Archive ; 041142-5
    ISBN: 3-540-48420-5
    Series Statement: Lecture Notes in Physics, 432
    Content: This book begins with a very readable survey "The Sun Today" by J.-C. Pecker. It is followed by thorough reviews from leading experts covering theory and observations. The focus shifts from the solar core, studied via neutrino emissions and helioseismology, through the interface regions where it is believed the large-scale magnetic fields are generated, to the corona, where most of the high temperature phenomena characteristic of this region may be studied directly. As energetic particles play such a vigorous role in this part of the sun, a separate session was devoted to their transport and storage in the corona.
    Note: Bibliographic Level Mode of Issuance: Monograph , The Sun today -- Recent results from helioseismology -- The structure of the solar core -- New sub-barrier nuclear fusion cross sections as a possible solution to the solar neutrino problem -- Helioseismic evidence for mixing in the radiative interior -- Microscopic settling and turbulent diffusion induced by rotation in the sun -- Mean-field theory of the solar dynamo -- Hydrodynamical simulations of the solar dynamo -- The asymmetric behaviour of solar activity -- On the possibility of supergiant stable flows in the convection zone of the sun -- Stellar dynamos -- On magnetic fields, rossby numbers and dynamo action in late-type stars -- The magnetic field of the solar corona -- The control of the corona by the convective zone magnetic fields -- Line-tying in a gravitationally stratified atmosphere -- Magnetic fields surrounding coronal holes -- Coronal heating mechanisms -- Coronal heating via nanoflares -- Magnetic structures of the intermediate corona -- Oscillations in quiescent prominences -- Pressure diagnostics of coronal loops observed by NIXT -- Quiet sun from multifrequency radio observations on RATAN-600 -- Frequency spectra of solar microwave bursts associated with coronal mass ejections -- Observations of high-energy (E?10 MeV) gamma-rays with the PHEBUS instrument -- Observational characteristics of explosive events -- Plasma physics of explosive phenomena -- A search for small solar flares with BATSE -- Solar flares and laboratory experiments -- Particle acceleration and radiation generation by nonlinear mode-mode coupling processes in the solar corona -- A fast mechanism for the acceleration of solar energetic particles in solar flares -- Acceleration and storage of energetic particles in the solar corona -- Electromagnetic signatures of particle acceleration and propagation -- Proton acceleration in long duration flares -- Signatures of proton beams in the Ly? profile: Sensitivity of the diagnostics -- Ground — based instrumentation -- Space instrumentation -- The Yohkoh mission: Instruments and recent results -- High resolution solar observations: Spectropolarimetry with THEMIS -- Conference summary. , English
    In: Springer eBooks
    Additional Edition: ISBN 3-540-58041-7
    Language: English
    DOI: 10.1007/3-540-58041-7
    URL: http://dx.doi.org/10.1007/3-540-58041-7
    Library Location Call Number Volume/Issue/Year Availability
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    Online Resource
    Open Access Request
    FU Berlin
  • 8
    Online Resource
    Online Resource
    Advances in Solar Physics : Proceedings of the Seventh European Meeting on Solar Physics Held in Catania, Italy, 11–15 May 1993 (1994)
    Berlin, Heidelberg :Springer Berlin Heidelberg,
    Details
    UID:
    almahu_9947923370302882
    Format: XVII, 338 p. , online resource.
    ISBN: 9783540484202
    Series Statement: Lecture Notes in Physics, 432
    Content: This book begins with a very readable survey "The Sun Today" by J.-C. Pecker. It is followed by thorough reviews from leading experts covering theory and observations. The focus shifts from the solar core, studied via neutrino emissions and helioseismology, through the interface regions where it is believed the large-scale magnetic fields are generated, to the corona, where most of the high temperature phenomena characteristic of this region may be studied directly. As energetic particles play such a vigorous role in this part of the sun, a separate session was devoted to their transport and storage in the corona.
    Note: The Sun today -- Recent results from helioseismology -- The structure of the solar core -- New sub-barrier nuclear fusion cross sections as a possible solution to the solar neutrino problem -- Helioseismic evidence for mixing in the radiative interior -- Microscopic settling and turbulent diffusion induced by rotation in the sun -- Mean-field theory of the solar dynamo -- Hydrodynamical simulations of the solar dynamo -- The asymmetric behaviour of solar activity -- On the possibility of supergiant stable flows in the convection zone of the sun -- Stellar dynamos -- On magnetic fields, rossby numbers and dynamo action in late-type stars -- The magnetic field of the solar corona -- The control of the corona by the convective zone magnetic fields -- Line-tying in a gravitationally stratified atmosphere -- Magnetic fields surrounding coronal holes -- Coronal heating mechanisms -- Coronal heating via nanoflares -- Magnetic structures of the intermediate corona -- Oscillations in quiescent prominences -- Pressure diagnostics of coronal loops observed by NIXT -- Quiet sun from multifrequency radio observations on RATAN-600 -- Frequency spectra of solar microwave bursts associated with coronal mass ejections -- Observations of high-energy (E?10 MeV) gamma-rays with the PHEBUS instrument -- Observational characteristics of explosive events -- Plasma physics of explosive phenomena -- A search for small solar flares with BATSE -- Solar flares and laboratory experiments -- Particle acceleration and radiation generation by nonlinear mode-mode coupling processes in the solar corona -- A fast mechanism for the acceleration of solar energetic particles in solar flares -- Acceleration and storage of energetic particles in the solar corona -- Electromagnetic signatures of particle acceleration and propagation -- Proton acceleration in long duration flares -- Signatures of proton beams in the Ly? profile: Sensitivity of the diagnostics -- Ground — based instrumentation -- Space instrumentation -- The Yohkoh mission: Instruments and recent results -- High resolution solar observations: Spectropolarimetry with THEMIS -- Conference summary.
    In: Springer eBooks
    Additional Edition: Printed edition: ISBN 9783540580416
    Language: English
    DOI: 10.1007/3-540-58041-7
    URL: http://dx.doi.org/10.1007/3-540-58041-7
    Library Location Call Number Volume/Issue/Year Availability
    BibTip Others were also interested in ...
    Online Resource
    Open Access Request
    HU Berlin
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